UBVRI polarimetry of the eclipsing binary V393 Cyg Antoniuk KA. UBVRI polarimetry of the eclipsing binary V393 Cyg. 2004 ;20(1):53-58.
The inclusion of magnetic splitting of lines in the determination of the lithium abundance and isotopic ratio in the atmosphere of the roAp-star HD 101065 1Shavrina AV, Khalack VR, Mykhailytska NG, Polosukhina NS. The inclusion of magnetic splitting of lines in the determination of the lithium abundance and isotopic ratio in the atmosphere of the roAp-star HD 101065. 2004 ;20(1):43-52.
Spectral investigations of the symbiotic star CH Cygni 1Mikailov KM, 1Khalilov VM. Spectral investigations of the symbiotic star CH Cygni. 2005 ;21(6):452-460.
Close binary systems in regions of OB-Associations. III. V443 Cygni in Cyg OB9 1Zakirov MM, 2Eshankulova MU. Close binary systems in regions of OB-Associations. III. V443 Cygni in Cyg OB9. 2005 ;21(6):441-451.
The structure of our stellar system 1Zakhozhay VA. The structure of our stellar system. 2005 ;21(6):414-440.
The study of gravitational fragmentation of colliding molecular clouds Vinogradov SB, Berczik PP. The study of gravitational fragmentation of colliding molecular clouds. 2005 ;21(5):368-388.
Nonspherical radiative supernova remnants Hnatyk B, Telezhinsky I. Nonspherical radiative supernova remnants. 2007 ;23(6):367-380.
Rapid variability of the He I λ 587.6 nm line in spectra of the Herbig Ae/Be WW Vul star Pugach AF. Rapid variability of the He I λ 587.6 nm line in spectra of the Herbig Ae/Be WW Vul star. 2007 ;23(4):222-229.
UVR CCD photometry of stars in five sky fields with matched IR/radio sources Kharin AS, Andruk VN, Bartasiute S, 1Butenko GZ, Vedenicheva IP, Perekhod AV, 1Sergeev AV. UVR CCD photometry of stars in five sky fields with matched IR/radio sources. 2007 ;23(4):207-221.
Transition of supernova remnants from adiabatic to radiative stage of evolution. Analytical approach Hnatyk B, Petruk O, Telezhinsky I. Transition of supernova remnants from adiabatic to radiative stage of evolution. Analytical approach. 2007 ;23(4):195-206.